A dataset provided by the European Space Agency

Name 014733
Title The missing soft X-ray luminosity in cluster cooling flows
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0147330101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0147330201

DOI 10.5270/esa-wln0yz5
Author Prof Andrew Fabian
Description Recent X-ray spectra of cluster cooling flows, particularly RGS spectra, have shown that the mass cooling rate is much smaller than previously estimated, with little emission seen from gas cooling below 1 keV. The expected soft X-ray luminosity is missing. Why the inner gas is so cool (20-30 per cent of the virial temperature) yet apparently not cooling is a puzzle, which has ramifications for galaxy formation. We propose deep RGS observations of A2597, A1835 and A1795 to resolve this important problem.
Publication An XMM-Newton observation of Abell 2597 . Morris, R. Glenn, Fabian, A. C., . MNRAS . 358-585 . 2005 . 2005MNRAS.358..585M ,
Metal abundances in the cool cores of galaxy clusters . de Grandi, S., Molendi, S., . A&A . 508-565 . 2009 . 2009A&A...508..565D ,
A revision of the X-ray absorption nature of BALQSOs . Streblyanska, A., Barcons, X., et all. . A&A . 515-2 . 2010 . 2010A&A...515A...2S ,
LoCuSS: A Herschel view of obscured star formation in Abell 1835 . Pereira, M. J., Haines, C. P., et all. . A&A . 518-40 . 2010 . 2010A&A...518L..40P ,
HIFLUGCS: Galaxy cluster scaling relations between X-ray luminosity, gas mass, cluster radius, and velocity dispersion . Zhang, Y.-Y., Andernach, H., et all. . A&A . 526-105 . 2011 . 2011A&A...526A.105Z ,
The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
The structural and scaling properties of nearby galaxy clusters. II. The M-T relation . Arnaud, M., Pointecouteau, E., . A&A . 441-893 . 2005 . 2005A&A...441..893A ,
The X-ray Energy Dependence of the Relation Between Optical and X-ray Emission in Quasars . Young, M., Elvis, M., . ApJ . 708-1388 . 2010 . 2010ApJ...708.1388Y ,
An Extremely Luminous Panchromatic Outburst ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-06-27T07:38:12Z/2003-07-30T20:05:30Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2004-10-26T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-10-26T00:00:00Z, 014733, 17.56_20190403_1200. https://doi.org/10.5270/esa-wln0yz5